Abstract The author discusses the relationship between X and radiation and radio to op-tical emission in blazars based on recent observations. The availability of densely-sampled light curves at several wavebands for several quasars, BL Lacertae, and two radio galaxies demonstrates that a strong connection exists between high and low frequency emission. The relativistic jet provides the most straightforward explanation of this connection. In the radio galaxies, temporary decreases in the X-ray flux from the central engine precede the appear-ance of bright superluminal knots in the radio jet. The combination of multiwaveband light curves and millimeter-wave imaging with very long baseline interferometry, along with po-larization measuremen...
Abstract Based on a sample of 69 blazars, relationships between flux density and spectral index, and...
Blazar spectra are one of the most important windows into the physical processes occurring along jet...
21 pages, 16 figures; Eq.B.2 and labels in few Figures correctedWe present models to predict high fr...
We study the correlation between the emission from the broad-line region (BLR) and the emission in o...
Blazars are a class of active galactic nuclei (AGN). Active galaxies are those that host compact sou...
Blazars, consisting of flat-spectrum radio quasars (FSRQs) and BL Lacertae objects (BL Lacs), are ac...
Blazars have their jet pointing towards us and are known for their emission that covers practically ...
Context. As a subcategory of active galactic nuclei, blazars are distinguished by their non-thermal ...
The extragalactic gamma-ray sky is largely dominated by radio-loud active galactic nuclei (AGN). In ...
Abstract In this paper, I discuss some historical data on the radio and X-ray variability of the act...
We present deep radio images at 1.4 GHz of a large and complete sample of BL Lacertae objects (BL La...
Abstract. The rich X-ray light curves of blazars obtained with RXTE allow meaningful correlation ana...
Blazars are active galactic nuclei characterized by ultra-luminous broad-band, non-thermal radio to ...
We present models to predict high-frequency counts of extragalactic radio sources using physically g...
Advances in the capabilities of X-ray, gamma-ray and TeV telescopes have brought new information on ...
Abstract Based on a sample of 69 blazars, relationships between flux density and spectral index, and...
Blazar spectra are one of the most important windows into the physical processes occurring along jet...
21 pages, 16 figures; Eq.B.2 and labels in few Figures correctedWe present models to predict high fr...
We study the correlation between the emission from the broad-line region (BLR) and the emission in o...
Blazars are a class of active galactic nuclei (AGN). Active galaxies are those that host compact sou...
Blazars, consisting of flat-spectrum radio quasars (FSRQs) and BL Lacertae objects (BL Lacs), are ac...
Blazars have their jet pointing towards us and are known for their emission that covers practically ...
Context. As a subcategory of active galactic nuclei, blazars are distinguished by their non-thermal ...
The extragalactic gamma-ray sky is largely dominated by radio-loud active galactic nuclei (AGN). In ...
Abstract In this paper, I discuss some historical data on the radio and X-ray variability of the act...
We present deep radio images at 1.4 GHz of a large and complete sample of BL Lacertae objects (BL La...
Abstract. The rich X-ray light curves of blazars obtained with RXTE allow meaningful correlation ana...
Blazars are active galactic nuclei characterized by ultra-luminous broad-band, non-thermal radio to ...
We present models to predict high-frequency counts of extragalactic radio sources using physically g...
Advances in the capabilities of X-ray, gamma-ray and TeV telescopes have brought new information on ...
Abstract Based on a sample of 69 blazars, relationships between flux density and spectral index, and...
Blazar spectra are one of the most important windows into the physical processes occurring along jet...
21 pages, 16 figures; Eq.B.2 and labels in few Figures correctedWe present models to predict high fr...